ASTR5590
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High Energy Astrophysics
Description
A core course intended for graduate students of Physics & Astronomy. This course explores high energy phenomena in a variety of astrophysical settings, including within diffuse plasmas and around compact objects. The physical processes producing radiation and particles will be introduced, and techniques for their detection in the X-ray, gamma ray, and cosmic ray regimes will be discussed. Topics include accretion disks, pulsars, non-magnetized neutron stars, binary X-ray sources, black holes, supernovae and supernova remnants, gamma ray bursts, gravitational wave sources, clusters of galaxies, and active galactic nuclei.
Minimum Credits
3
Maximum Credits
3
Repeat for Credit
No
Required Requisite(s):
007835
Course Attributes
HON - HON (Honors)
Semesters Typically Offered
Fall Even Year